Canl\u0131l\u0131k konusu, asl\u0131nda d\u00fcnyayla s\u0131n\u0131rl\u0131 bir olgu de\u011fildir. Genel anlamda canl\u0131l\u0131k konusu evrensel bir olgudur. Bunu d\u00fcnya gibi, evrende toz zerresi kadar olan bir uzaysal obje ile s\u0131n\u0131rlamak \u00e7ok dar bir g\u00f6r\u00fc\u015f olur. \u00c7\u00fcnk\u00fc bug\u00fcne kadar yap\u0131lan ara\u015ft\u0131rmalar\u0131n sonucunda elde edilen bilgiler, belgeler, g\u00f6zlemler ve ara\u015ft\u0131rmalar bunu s\u00f6ylemektedir.<\/p>\n
K\u0131saca uzaysal bilgilerimizi hat\u0131rlayacak olursak Galaktik \u00f6l\u00e7\u00fcleri veya G\u00fcne\u015f sistemi ile ilgili \u00f6l\u00e7\u00fcleri g\u00f6z \u00f6n\u00fcne getirirsek bir de d\u00fcnyan\u0131n boyutlar\u0131n\u0131 g\u00f6z \u00f6n\u00fcnde tutarsak g\u00f6r\u00fcr\u00fcz ki, \u015fu an \u00fczerinde ya\u015fad\u0131\u011f\u0131m\u0131z d\u00fcnya gezegeni bu boyutlar \u00f6l\u00e7\u00fcs\u00fcnde hemen hemen hi\u00e7 durumunda kalmaktad\u0131r. Dolay\u0131s\u0131yla bu k\u00fc\u00e7\u00fcc\u00fck \u00f6l\u00e7\u00fcler i\u00e7ine canl\u0131l\u0131k gibi evrensel bir olguyu s\u0131\u011fd\u0131rmak, s\u0131k\u0131\u015ft\u0131rmak ne kadar do\u011fru olur?<\/p>\n
\u00c7\u00fcnk\u00fc \u015fu anda d\u00fcnya d\u0131\u015f\u0131 canl\u0131l\u0131kla ilgili pek \u00e7ok belge, g\u00f6zlem, ara\u015ft\u0131rma ve hatta tarihsel bulgular bulunmaktad\u0131r. Bu bilgiler \u0131\u015f\u0131\u011f\u0131nda ortaya \u00e7\u0131kan sonu\u00e7 Evrende yaln\u0131z olmad\u0131\u011f\u0131m\u0131z y\u00f6n\u00fcndedir. D\u00fcnya d\u0131\u015f\u0131 canl\u0131l\u0131k konusu bir olas\u0131l\u0131k de\u011fildir. D\u00fcnya d\u0131\u015f\u0131 canl\u0131l\u0131\u011f\u0131n yayg\u0131nl\u0131\u011f\u0131 s\u00f6z konusudur. Evrenlere da\u011f\u0131lm\u0131\u015f olmas\u0131 s\u00f6z konusudur. Hatta \u00e7ok de\u011fi\u015fik \u015fuur d\u00fczeylerindeki varl\u0131klar evrenlere yay\u0131lm\u0131\u015f vaziyettedir.<\/p>\n
D\u00fcnya d\u0131\u015f\u0131 canl\u0131l\u0131k yani bilimsel ad\u0131yla Egzobiyoloji konusunda yap\u0131lan ara\u015ft\u0131rmalar\u0131 3 ana ba\u015fl\u0131k alt\u0131nda incelemek m\u00fcmk\u00fcnd\u00fcr.<\/p>\n
1-\u00a0 Meteorlarla ilgili ara\u015ft\u0131rmalar<\/p>\n
2- Yapay atmosfer ara\u015ft\u0131rmalar\u0131<\/p>\n
3- Radyoteleskoplarla yap\u0131lan Y\u0131ld\u0131z dinleme operasyonlar\u0131<\/p>\n
Meteorlarla ilgili ara\u015ft\u0131rmalar\u0131 \u015fu \u015fekilde \u00f6zetleyebiliriz.<\/p>\n
Yap\u0131lan ara\u015ft\u0131rmalar sonucunda, uzaydan d\u00fcnyam\u0131za s\u00fcrekli olarak meteor ya\u011fmurlar\u0131 oldu\u011fu g\u00f6r\u00fclmektedir. Dolay\u0131s\u0131yla d\u00fcnyam\u0131za d\u0131\u015f uzaydan baz\u0131 partik\u00fcller gelmektedir. Bunlar\u0131n \u00fczerinde yap\u0131lan ara\u015ft\u0131rmalar sonucunda bilim adamlar\u0131 organizma sporlar\u0131na rastlam\u0131\u015flard\u0131r. Aminoasitlere, Ya\u011f asitlerine, Hidrokarbonlara ve organik bile\u015fiklere rastlam\u0131\u015flard\u0131r. Hatta Meteoritlerden bir k\u00fclt\u00fcr bile olu\u015fturulmu\u015ftur.<\/p>\n
Yapay Atmosfer ara\u015ft\u0131rmalar\u0131, 1953 y\u0131l\u0131nda Stanley Miller adl\u0131 bir bilim adam\u0131n\u0131n d\u00fcnyan\u0131n olu\u015fumu s\u0131ras\u0131ndaki atmosferini laboratuvar ortam\u0131nda yapay olarak meydana getirmesiyle ba\u015flam\u0131\u015ft\u0131r. Bu atmosferin i\u00e7erdi\u011fi maddeler \u015funlardan olu\u015fmaktad\u0131r. Metan, Su buhar\u0131, Amonyak, Karbondioksit ve Siyanhidrik asit bile\u015fikleri.<\/p>\n
G\u00f6r\u00fcld\u00fc\u011f\u00fc gibi bunlar\u0131n hepsi, su buhar\u0131 hari\u00e7 \u015fu anda bizler (canl\u0131lar) i\u00e7in zehir durumundad\u0131r. G\u00f6r\u00fcld\u00fc\u011f\u00fc gibi d\u00fcnyada canl\u0131l\u0131k, \u015fu an bizler i\u00e7in zehir say\u0131labilecek bir ortamda ba\u015flam\u0131\u015ft\u0131r. Yap\u0131lan bu ara\u015ft\u0131rmalar sonucunda; Evrende canl\u0131l\u0131\u011f\u0131n, yani hayat\u0131n meydana gelebilmesi i\u00e7in suyun ve oksijenin \u015fart olmad\u0131\u011f\u0131n\u0131 s\u00f6yleyebiliriz.<\/p>\n
Radyoteleskoplarla ilgili ara\u015ft\u0131rmalar\u0131n ba\u015f\u0131nda ise, 1960\u2019larda Amerika\u2019n\u0131n \u00f6nemli astronomlar\u0131ndan biri olan Prof. Frank Drake taraf\u0131ndan ba\u015flat\u0131lm\u0131\u015f olan Ozma Projesi vard\u0131. Projede o zaman\u0131n radyoteleskoplar\u0131yla uzaysal objeden gelen sinyal tipleri dinlenmeye ba\u015fland\u0131.<\/p>\n
Bunun uzant\u0131s\u0131 olarak g\u00fcn\u00fcm\u00fczde de hala SET\u0130 (Search for Extra Terrestrial Inteligence ) D\u00fcnya D\u0131\u015f\u0131 Ya\u015fam\u0131 Ara\u015ft\u0131rma Projesi s\u00fcrd\u00fcr\u00fclmektedir. SET\u0130 projesinin arkas\u0131nda bug\u00fcn NASA destekli olmak \u00fczere Planetary Society bulunmaktad\u0131r. Ve bu ara\u015ft\u0131rmalar g\u00fcn\u00fcm\u00fczde de y\u0131ld\u0131z dinleme projesi olarak devam etmektedir.<\/p>\n
Bu \u00e7al\u0131\u015fmalar\u0131n paralelini Rusyada da g\u00f6rmekteyiz. \u00d6rne\u011fin; Gorki g\u00f6zlemevi m\u00fcd\u00fcr\u00fc Prof. Vesvolod Troitsky, \u201cBa\u015fka medeniyetlerin bizi elektromanyetik dalgalarla tarad\u0131\u011f\u0131na kuvvetle inan\u0131yoruz. Bunun sonu\u00e7lar\u0131n\u0131 er ya da ge\u00e7 alaca\u011f\u0131z\u201d demektedir.<\/p>\n
Prof. Troitsky\u2019nin belirtti\u011fine g\u00f6re, Kuzey Kafkasya Da\u011flar\u0131\u2019nda 1973 y\u0131l\u0131nda yeni ve b\u00fcy\u00fck bir g\u00f6zlemevi a\u00e7\u0131lm\u0131\u015ft\u0131r. Bu g\u00f6zlemevinin optik teleskobu Palomar Da\u011f\u0131\u2019ndak\u0130 200 in\u00e7lik teleskoptan daha b\u00fcy\u00fckt\u00fcr. Radyoteleskobu ise 2000 feet \u00e7ap\u0131ndad\u0131r. Bu iki teleskop zeki sinyallerin saptanmas\u0131 \u00e7al\u0131\u015fmalar\u0131nda d\u00f6n\u00fc\u015f\u00fcml\u00fc olarak kullan\u0131lmaktad\u0131r.<\/p>\n
Moskova Devlet \u00dcniversitesi Radyo Astronomi Direkt\u00f6r\u00fc olan Prof. Josif Shklovsky ise d\u00fcnya d\u0131\u015f\u0131 bir medeniyetle temas\u0131n \u00e7ok yak\u0131n oldu\u011funu ifade etmektedir. T\u00fcm bu geli\u015fmelerin paralelinde d\u00fcnyan\u0131n \u00e7e\u015fitli \u00fcniversitelerinde de konuyu incelemek amac\u0131yla \u201cEgzobiyoloji\u201d ad\u0131 alt\u0131nda d\u00fcnya d\u0131\u015f\u0131 hayat\u0131 ara\u015ft\u0131ran k\u00fcrs\u00fcler kurulmu\u015ftur.<\/p>\n
Bunlara \u00f6rnek olarak: Alabama, Missisipi, Hamburg, Kiel, Utretch, Mainz, Boston \u00dcniversiteleriyle Edison Sommunity, Moorpark Junior, Victor Halley ve Londra\u2019da ki Marley Koleji\u2019ni g\u00f6sterebiliriz.<\/p>\n
Evrende zeki hayat konusunda astronomlar\u0131n matematiksel hesaplamalar\u0131na g\u00f6re \u00d6rne\u011fin: Astronom Harlow Shapley\u2019e g\u00f6re teleskoplar\u0131n g\u00f6r\u00fc\u015f alan\u0131 i\u00e7inde (100 Katrilyon) adet y\u0131ld\u0131z bulunmaktad\u0131r.<\/p>\n
Bu y\u0131ld\u0131zlar\u0131n binde birinde hayat i\u00e7in elveri\u015fli ko\u015fullar\u0131n bulundu\u011funu kabul etti\u011fimizde, geriye (100 Trilyon) adet y\u0131ld\u0131z\u0131n kald\u0131\u011f\u0131n\u0131 s\u00f6ylemektedir. Bunlar\u0131n binde birinde hayata uygun atmosferin bulundu\u011funu farz edersek, geriye (100 Milyar) adet y\u0131ld\u0131z\u0131n bulunabilece\u011fini ileri s\u00fcrmektedir.<\/p>\n
Astronom Harlow Shapley, daha da ileri giderek, bunlar\u0131n da binde birinde hayat\u0131n ortaya \u00e7\u0131kabilece\u011fini kabul edersek, \u015fu anda \u00fczerinde hayat olan gezegen say\u0131s\u0131 (100 Milyon) adettir. Isaac Asimov, \u201cSadece galaksimiz Samanyolu\u2019ndaki ya\u015fanabilir gezegenlerin say\u0131s\u0131n\u0131n 650 Milyon olmas\u0131 gerekti\u011fini hesaplam\u0131\u015ft\u0131r. Bu sonuca g\u00f6re en az\u0131ndan g\u00f6zlenebilir evrenin t\u00fcm\u00fcnde, 2 Milyar adet ya\u015fanabilir gezegen bulunmaktad\u0131r\u201d demektedir.<\/p>\n
EVRENDE ZEKi HAYATIN B\u0130L\u0130MSEL KANITLARI<\/span><\/strong><\/p>\n NASA, A\u011fustos 1989\u2019da insans\u0131z uzay arac\u0131 Voyager 2\u2019yle Nept\u00fcn gezegenin yan\u0131ndan ge\u00e7ti ve d\u00fcnyaya resimler ve \u00e7e\u015fitli veriler yollad\u0131. Bu ara\u00e7 d\u00fcnyaya \u0131\u015f\u0131k h\u0131z\u0131nda bile varmas\u0131 4 saat s\u00fcren darbe sesleri yollad\u0131. Bu darbeler d\u00fcnya \u00fczerinde NASA\u2019n\u0131n uzay a\u011f\u0131n\u0131 olu\u015fturan radyoteleskoplar\u0131 arac\u0131l\u0131\u011f\u0131yla yakaland\u0131 ve sonra zay\u0131f sinyaller Pasadena \/ California\u2019da bulunan NASA\u2019n\u0131n Jet \u00eetki Laboratuvar\u0131n\u0131n geli\u015fmi\u015f tesislerinde elektronik sihirbazl\u0131k yoluyla foto\u011fraflara, tablolara ve di\u011fer veri bi\u00e7imlerine \u00e7evrildi.<\/p>\n Nept\u00fcn ziyaretinden 12 y\u0131l \u00f6nce A\u011fustos 1977\u2019de f\u0131rlat\u0131lan Voyager 2 ve refakat\u00e7isi Voyager l\u2019in asl\u0131nda sadece J\u00fcpitere ve Sat\u00fcrn\u2019e ula\u015fmas\u0131 ve daha \u00f6nce Pioneer 10 ve Pioneer 11 adl\u0131 insans\u0131z uzay ara\u00e7lar\u0131 taraf\u0131ndan bu iki dev gaz\u0131ms\u0131 gezegen hakk\u0131nda elde edilen verileri art\u0131rmas\u0131 niyetleniyordu.<\/p>\n Ama kayda de\u011fer bir deha ve beceri ile JPL bilimcileri ve teknisyenleri, d\u0131\u015f gezegenlerin nadir bir \u015fekilde hizaya girmesinden faydalanarak ve bu gezegenlerin yer\u00e7ekimi g\u00fc\u00e7lerini \u201csapan\u201d gibi kullanarak Voyager 2\u2019yi ilk \u00f6nce Sat\u00fcrn\u2019den Uran\u00fcs\u2019e sonra da Uran\u00fcs\u2019ten Nept\u00fcn\u2019e f\u0131rlatmay\u0131 ba\u015fard\u0131lar.<\/p>\n Voyager 2 den gelen elektronik sinyaller Helyum, hidrojen ve metan gazlar\u0131ndan olu\u015fan bir atmosferin kucaklad\u0131\u011f\u0131, d\u00fcnyan\u0131n kas\u0131rgalar\u0131n\u0131 k\u00fc\u00e7\u00fcc\u00fck k\u0131lan, burga\u00e7l\u0131, y\u00fcksek \u015fiddette r\u00fczg\u00e2rlar\u0131n s\u00fcp\u00fcrd\u00fc\u011f\u00fc g\u00fczel bir mavi-ye\u015fil renge sahip, turkuaz bir gezegeni a\u00e7\u0131\u011fa \u00e7\u0131kard\u0131lar. Beklendi\u011fi gibi atmosfer ve y\u00fczey \u0131s\u0131lar\u0131 donma noktas\u0131n\u0131n alt\u0131ndayd\u0131 ama Nept\u00fcn\u2019\u00fcn, beklenmedik bi\u00e7imde, gezegen i\u00e7inden \u00e7\u0131kan bir \u0131s\u0131 yayd\u0131\u011f\u0131 bulundu.<\/p>\n Nept\u00fcn\u2019\u00fcn bir gaz devi oldu\u011fu yolundaki daha \u00f6nceki fikirlerin aksine gezegenin, JPL bilimcilerinin kelimeleriyle, \u00fcst\u00fcnde \u201csu buzundan olu\u015fan yar\u0131 erimi\u015f bir kar\u0131\u015f\u0131m\u0131n y\u00fczd\u00fc\u011f\u00fc kayal\u0131k bir \u00e7ekirde\u011fe sahip oldu\u011fu, Voyager 2 taraf\u0131ndan belirlendi. Nept\u00fcn\u2019\u00fcn 8 uydusu oldu\u011fu saptand\u0131. Ve bu uydular\u0131n en b\u00fcy\u00fc\u011f\u00fcne Triton ad\u0131 verildi.<\/p>\n Triton\u2019un yap\u0131s\u0131 da Nept\u00fcn gezegenine benziyordu. Yak\u0131n plan resimleri \u00e7ok garip bir t\u00fcrden volkanik aktivite oldu\u011funu \u00f6nermekteydi. G\u00f6k cisminin aktif, s\u0131cak i\u00e7 k\u0131sm\u0131n\u0131n d\u0131\u015far\u0131ya p\u00fcsk\u00fcrten erimi\u015f lavlar de\u011fil, sulu buz f\u0131skiyeleri oldu\u011fu ortaya \u00e7\u0131kt\u0131. Haz\u0131rl\u0131k a\u015famas\u0131ndaki de\u011ferlendirmeler Triton\u2019un ge\u00e7mi\u015finde y\u00fczeyde akan sular oldu\u011funu, hatta jeolojik \u00f6l\u00e7e\u011fe g\u00f6re nispeten yak\u0131n zamana kadar y\u00fczeyde g\u00f6ller bile oldu\u011funu belirtmekteydi.<\/p>\n NASA, Voyager 2 uydusu arac\u0131l\u0131\u011f\u0131yla Uran\u00fcs\u2019\u00fcn de gazlarla de\u011fil sularla kapl\u0131 oldu\u011funu ve y\u00fczeyinde sadece bir donmu\u015f su katman\u0131 de\u011fil, bir su okyanusu oldu\u011funu ortaya \u00e7\u0131kard\u0131. Daha sonra Voyager 2, Uran\u00fcs\u2019\u00fcn aylar\u0131n\u0131n da kayadan ve s\u0131radan su buzundan olu\u015ftu\u011funu bulmu\u015ftu.<\/p>\n NASA, 1974 \/ 1975\u2019te uzaya g\u00f6nderilen Mariner 10 adl\u0131 insans\u0131z uzay arac\u0131n\u0131n d\u00fcnyaya g\u00f6nderdi\u011fi foto\u011fraflarda Mars\u0131n y\u00fczeyinin su buhar\u0131yla kapl\u0131 oldu\u011funu g\u00f6sterdi.<\/p>\n Aral\u0131k 1978\u2019den sonra Pioneer-Ven\u00fcs l ve 2 adl\u0131 iki insans\u0131z uzay arac\u0131 taraf\u0131ndan Ven\u00fcs\u2019\u00fcn uzun s\u00fcre incelenmesiyle elde edilen veriler, bulgular\u0131 analiz eden bilimcilerden olu\u015fan ekipleri, Ven\u00fcs\u2019\u00fcn \u201cbir zamanlar en az\u0131ndan ortalama 10 metre derinli\u011finde suyla kapl\u0131 olabilece\u011fi\u201d konusunda ikna etmi\u015ftir. Ven\u00fcs, diye sonuca vard\u0131lar.<\/p>\n Bug\u00fcn buhar halinde sahip oldu\u011fu suyun en az\u0131ndan 100 kat\u0131na, bir zamanlar su olarak sahipti.\u201d Ard\u0131ndan gelen \u00e7al\u0131\u015fmalar bu kadim suyun bir b\u00f6l\u00fcm\u00fcn\u00fcn s\u00fclf\u00fcrik asit bulutlar\u0131n\u0131 olu\u015fturmakta kullan\u0131ld\u0131\u011f\u0131n\u0131n, bir k\u0131sm\u0131n\u0131n da gezegenin kayal\u0131k y\u00fczeyini okside etmek \u00fczere oksijeninden vazge\u00e7ti\u011fini \u00f6nermekteydi.<\/p>\n NASA, Viking 2 insans\u0131z uzay arac\u0131n\u0131n durdu\u011fu yerdeki zeminde don oldu\u011funu bildirmi\u015fti. Don tabakas\u0131n\u0131n su, su buzu ve donmu\u015f karbondioksit (kuru buz) i\u00e7erdi\u011fi bulunmu\u015ftur. Mars\u2019\u0131n kutuplar\u0131ndaki buz tabakalar\u0131n\u0131n su buzu ya da kuru buz i\u00e7erip i\u00e7ermedi\u011fi tart\u0131\u015fmas\u0131 NASA\u2019n\u0131n JPL bilimcilerinin Pasadena\u2019daki (Caltech) California Teknoloji Enstit\u00fcs\u00fcnde Ocak 1979\u2019da d\u00fczenlenen 2. Uluslararas\u0131 Mars toplant\u0131s\u0131nda g\u00fcney kutbu de\u011fil ama \u201ckuzey kutbu su buzu i\u00e7ermektedir\u201d diye a\u00e7\u0131klama yapmalar\u0131yla sonuca ba\u011fland\u0131.<\/p>\n D\u00fcnyam\u0131zdan 800 kat daha b\u00fcy\u00fck olan Sat\u00fcrn\u2019\u00fcn y\u00fczeyine hen\u00fcz n\u00fcfuz edilemedi. Pioneer 11 1979\u2019da Sat\u00fcrn\u2019\u00fcn halkalar\u0131n\u0131n ve Aylar\u0131n\u0131n b\u00fcy\u00fck \u00f6l\u00e7\u00fcde olmasa bile, su buzundan ve hatta belki de s\u0131v\u0131 sudan olu\u015ftu\u011funu ortaya \u00e7\u0131kartm\u0131\u015ft\u0131r.<\/p>\n J\u00fcpiter, Pioneer 10 \u2013 Pioneer 11 ve Voyager tarafindan incelendi. Sonu\u00e7lar Sat\u00fcrn\u2019dekilerden pek farkl\u0131 de\u011fildir. Gaz devi gezegenin \u00e7ok b\u00fcy\u00fck miktarlarda radyasyon ve \u0131s\u0131 yayd\u0131\u011f\u0131 ve \u015fiddetli f\u0131rt\u0131nalara tabi olan kal\u0131n bir atmosferle sarmaland\u0131\u011f\u0131 bulundu.<\/p>\n Ancak bu n\u00fcfuz edilemez \u00f6rt\u00fcn\u00fcn, esasen hidrojen, helyum, metan, amonyak, su buhar\u0131 ve muhtemelen su damlac\u0131klar\u0131ndan olu\u015ftu\u011fu bulundu, bilim adamlar\u0131, bu kal\u0131n atmosferin daha da a\u015fa\u011f\u0131lar\u0131nda bir yerlerde s\u0131v\u0131 suyun oldu\u011fu sonucuna vard\u0131lar. J\u00fcpiter\u2019in aylar\u0131n\u0131n da su buhar\u0131 ve su damlac\u0131klar\u0131 ile kapl\u0131 oldu\u011fu sonucuna vard\u0131lar. \u00d6zellikle lo, Europa, Ganymede ve Callisto uydular\u0131d\u0131r.<\/p>\n UFO NED\u0130R?<\/span><\/strong><\/p>\n UFO (Unidentif\u0131ed Flying Object \u2013 Tan\u0131mlanamayan U\u00e7an Nesne) terimi ilk olarak ABD Hava Kuvvetleri\u2019nde Y\u00fczba\u015f\u0131 olan Edward James Ruppelt tarafindan kullan\u0131lm\u0131\u015ft\u0131r. Y\u00fczba\u015f\u0131 Ruppelt 1951 y\u0131l\u0131nda bu fenomenlerle ilgili olarak Hava Kuvvetlerinde bir ara\u015ft\u0131rma y\u00fcr\u00fctmekteydi. Ruppelt\u2019in ara\u015ft\u0131rmas\u0131ndan \u00f6nce UFO\u2019lara (Flying Saucers \u2013 U\u00e7an \u00c7ay Tabaklar\u0131) ad\u0131 veriliyordu.<\/p>\n \u00c7\u00fcnk\u00fc bir\u00e7ok g\u00f6rg\u00fc tan\u0131\u011f\u0131 bu nesneleri daire \u015feklinde tasvir ediyordu. Ancak \u201cU\u00e7an \u00c7ay Tabaklar\u0131\u201d terimi \u00e7ok say\u0131da gazete ve dergi yazar\u0131n\u0131n g\u00f6sterdi\u011fi ku\u015fkuculuk nedeniyle k\u0131sa s\u00fcrede alay konusu oldu. Y\u00fczba\u015f\u0131 Ruppelt ise s\u00fcrd\u00fcrd\u00fc\u011f\u00fc ara\u015ft\u0131rmaya sayg\u0131nl\u0131k kazand\u0131rmak amac\u0131yla \u201cTan\u0131mlanamayan U\u00e7an Nesne\u201d terimini kulland\u0131. UFO terimi, daha belirgin bir niteli\u011fe sahipti. \u00c7\u00fcnk\u00fc tan\u0131mlanamayan u\u00e7an nesnelerin hepsi tabak \u015feklinde de\u011fildi.<\/p>\n Her y\u0131l polise, bas\u0131n organlar\u0131na veya UFO ara\u015ft\u0131rma gruplar\u0131na binlerce UFO olay\u0131 aktar\u0131l\u0131r. Bu raporlar UFO\u2019lar\u0131n ger\u00e7ekte k\u00fc\u00e7\u00fck bir az\u0131nl\u0131\u011f\u0131n\u0131 olu\u015fturmaktad\u0131r. \u00c7\u00fcnk\u00fc UFO tan\u0131klar\u0131n\u0131n \u00e7o\u011fu bu kar\u015f\u0131la\u015fmalar\u0131 kamuoyuna a\u00e7\u0131klamaz.<\/p>\n Rapor edilen UFO\u2019lar\u0131n kabaca % 90 \u2013 95\u2019inin insan yap\u0131m\u0131 u\u00e7ak veya bilinmeyen do\u011fa olaylar\u0131 oldu\u011fu kan\u0131tlanm\u0131\u015ft\u0131r. Yakla\u015f\u0131k % 1,5 \u2013 2\u2019si ise, genellikle fotomontaj foto\u011fraflardan \u00fcretilmi\u015f hilelerden olu\u015fmaktad\u0131r.<\/p>\n Bu hileler a\u015f\u0131r\u0131 miktarda sorun yaratmaktad\u0131r. UFO g\u00f6zlemlerinin geri kalan % 3 \u2013 8,5\u2019i ise, insan \u00fcr\u00fcn\u00fc olmayan bir kayna\u011fa sahip hava ta\u015f\u0131t\u0131 gibi g\u00f6r\u00fcnmektedir. Ara\u015ft\u0131rmac\u0131lar\u0131n \u00e7o\u011fu da bu son gruba girenlerle ilgilenmektedir.<\/p>\n Kaynak; Adana Ruhsal Ara\u015ft\u0131rmalar Derne\u011fi<\/p>\n","protected":false},"excerpt":{"rendered":" Canl\u0131l\u0131k konusu, asl\u0131nda d\u00fcnyayla s\u0131n\u0131rl\u0131 bir olgu de\u011fildir. Genel anlamda canl\u0131l\u0131k konusu evrensel bir olgudur. Bunu d\u00fcnya gibi, evrende toz zerresi kadar olan bir uzaysal obje ile s\u0131n\u0131rlamak \u00e7ok dar bir g\u00f6r\u00fc\u015f olur. \u00c7\u00fcnk\u00fc bug\u00fcne kadar yap\u0131lan ara\u015ft\u0131rmalar\u0131n sonucunda elde edilen bilgiler, belgeler, g\u00f6zlemler ve ara\u015ft\u0131rmalar bunu s\u00f6ylemektedir. K\u0131saca uzaysal bilgilerimizi hat\u0131rlayacak olursak Galaktik \u00f6l\u00e7\u00fcleri …<\/p>\n","protected":false},"author":1,"featured_media":306,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[2],"tags":[],"class_list":["post-305","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-dunya-disi"],"_links":{"self":[{"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/posts\/305","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/comments?post=305"}],"version-history":[{"count":2,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/posts\/305\/revisions"}],"predecessor-version":[{"id":2568,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/posts\/305\/revisions\/2568"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/media\/306"}],"wp:attachment":[{"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/media?parent=305"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/categories?post=305"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/kosmosmacerasi.com\/v1\/wp-json\/wp\/v2\/tags?post=305"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}